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astronomy

NGC 7316

NGC 7316 is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand NGC 7316 rather than just read about it. In short: NGC 7316 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 5,198±25 km/s, which corresponds to a Hubble distance of 250.1 ± 17.5 Mly (76.67 ± 5.38 Mpc).

NGC 7316 — main illustration
NGC 7316 — illustration

Key takeaways

  • NGC 7316 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect NGC 7316 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 7316 from memory before moving on to harder problems.

Reference excerpt

NGC 7316 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 5,198±25 km/s, which corresponds to a Hubble distance of 250.1 ± 17.5 Mly (76.67 ± 5.38 Mpc). However, three non-redshift measurements give a closer mean distance of 212.87 ± 3.89 Mly (65.267 ± 1.192 Mpc). It was discovered by German-British astronomer William Herschel on 18 September 1784. NGC 7316 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. NGC 7316 is also a starburst galaxy. NGC 7316 has a nucleus with excessive amounts of ultraviolet emissions compared with other galaxies, and is listed in the Markarian catalogue as MRK 307.

Galaxy group According to M. J. Geller and J. P. Huchra, NGC 7316 is a member of a galaxy group which contains 2 other galaxies: NGC 7321 and NGC 7323.

Supernovae Two supernovae have been observed in NGC 7316:

SN 2006cx (Type II, mag. 17.4) was discovered by the Lick Observatory Supernova Search (LOSS) on 8 June 2006. SN 2016hvu (Type II-P, mag. 17.6) was discovered by the Catalina Real-time Transient Survey on 6 November 2016.

See also List of NGC objects (7001–7840)

References

External links Media related to NGC 7316 at Wikimedia Commons NGC 7316 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 7316 illustration

Worked examples

Example 1 — a first encounter with NGC 7316

Start with the simplest possible case. Write down what NGC 7316 claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to NGC 7316 before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about NGC 7316 ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of NGC 7316

In research
NGC 7316 appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses NGC 7316 in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
NGC 7316 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1784, Barred spiral galaxies, Discoveries by William Herschel, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 7316 outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.

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How to study NGC 7316 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 7316 means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain NGC 7316 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 7316 in simple terms?

NGC 7316 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 5,198±25 km/s, which corresponds to a Hubble distance of 250.1 ± 17.5 Mly (76.67 ± 5.38 Mpc).

Why does NGC 7316 matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study NGC 7316?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on NGC 7316.

Tags

  • Astronomical objects discovered in 1784
  • Barred spiral galaxies
  • Discoveries by William Herschel
  • IRAS catalogue objects
  • MCG objects
  • Markarian galaxies
  • NGC objects
  • Pegasus (constellation)
  • Principal Galaxies Catalogue objects
  • UGC objects

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